A Reference Sample: ISM of the Most Isolated Galaxies
L. Verdes‐Montenegro(Instituto de Astrofísica de Andalucía), F. Combes(Observatoire de Paris), D. Espada(The Graduate University for Advanced Studies, SOKENDAI), Min S. Yun(University of Massachusetts Amherst), W. K. Huchtmeier(Max Planck Institute for Radio Astronomy), U. Lisenfeld(Instituto de Radioastronomía Milimétrica), S. C. Odewahn, S. Del Rio(National Institute of Astrophysics, Optics and Electronics), J. W. Sulentic(Instituto de Astrofísica de Andalucía), E. García(Instituto de Astrofísica de Andalucía), S. Léon(Instituto de Radioastronomía Milimétrica), S. Verley(Universidad de Granada)
Cited by 0
Related Papers
High molecular gas fractions in normal massive star-forming galaxies in the young Universe
|Nature|2010|991
A study of the gas-star formation relation over cosmic time★
|Monthly Notices of the Royal Astronomical Society|2010|952
PHIBSS: MOLECULAR GAS CONTENT AND SCALING RELATIONS IN<i>z</i>∼ 1-3 MASSIVE, MAIN-SEQUENCE STAR-FORMING GALAXIES
|The Astrophysical Journal|2013|941
A Catalog of Neighboring Galaxies
|The Astronomical Journal|2004|829